LINK<\/strong><\/a><\/p>\n\n\n\n“Highlights<\/p>\n\n\n\n
\u2022 We obtained Al\u2013Mg mineral isochrons of three CAIs primarily formed by condensation.
\n\u2022 Inferred (26Al\/27Al)0 range from (5.19 \u00b1 0.17) to (4.39 \u00b1 0.08) \u00d7 10\u22125.
\n\u2022 The spread of (26Al\/27Al)0 is similar to that for igneous CAIs in CV chondrites.
\n\u2022 This infers that the CAI melting and condensation continued for at least \u223c0.2 Myr.
\n\u2022 It would also imply heterogeneous distributions of 26Al in the forming region.”<\/p>\n\n\n\n
“Al\u2013Mg mineral isochrons of three Ca\u2013Al-rich inclusions (CAIs) that formed primarily by condensation, one fine-grained, spinel-rich inclusion and two fluffy Type A CAIs, from the reduced CV chondrites Efremovka and Vigarano were obtained by in situ Al\u2013Mg isotope measurements using secondary ion mass spectrometry. The slope of the isochron obtained for the fine-grained, spinel-rich inclusion gives an initial 26Al\/27Al value, (26Al\/27Al)0, of (5.19 \u00b1 0.17) \u00d7 10\u22125. This is essentially identical to the Solar System initial 26Al\/27Al determined by whole-rock Al\u2013Mg isochron studies for CAIs in CV chondrites. In contrast, the isochron slopes for the two fluffy Type A CAIs from their Al\u2013Mg mineral isochrons, (4.703 \u00b1 0.082) \u00d7 10\u22125 and (4.393 \u00b1 0.084) \u00d7 10\u22125, are significantly lower than the Solar System initial value. The range of (26Al\/27Al)0 values of the three CAIs, from (5.19 \u00b1 0.17) to (4.393 \u00b1 0.084) \u00d7 10\u22125, corresponds to a formation age spread of 0.17 \u00b1 0.04 Myr. This formation age spread is similar to that of igneous CAIs from CV chondrites. The data suggest that condensation and melting of minerals occurred in the hot nebular gas contemporaneously for \u223c0.2 Myr at the very beginning of our Solar System, if 26Al was distributed homogeneously in the CAI forming region. Alternatively, the observed variations in (26Al\/27Al)0 among fluffy Type A CAIs would also raise a possibility of heterogeneous distributions of 26Al in the forming region.”<\/p>\n","protected":false},"excerpt":{"rendered":"
Noriyuki Kawasaki, Changkun Park, Naoya Sakamoto, Sun Young Park, Hyun Na Kim, Minami Kuroda, Hisayoshi Yurimoto Earth and Planetary Science Letters Volume 511, 1 April 2019, Pages 25-35 LINK “Highlights \u2022 We obtained Al\u2013Mg mineral…<\/p>\n","protected":false},"author":1,"featured_media":0,"comment_status":"closed","ping_status":"closed","sticky":false,"template":"","format":"standard","meta":{"footnotes":""},"categories":[66,9,14,22,57,2531],"tags":[238,448,3830,3006,3273,1812,2401,4147,675],"_links":{"self":[{"href":"https:\/\/karmaka.de\/index.php?rest_route=\/wp\/v2\/posts\/17329"}],"collection":[{"href":"https:\/\/karmaka.de\/index.php?rest_route=\/wp\/v2\/posts"}],"about":[{"href":"https:\/\/karmaka.de\/index.php?rest_route=\/wp\/v2\/types\/post"}],"author":[{"embeddable":true,"href":"https:\/\/karmaka.de\/index.php?rest_route=\/wp\/v2\/users\/1"}],"replies":[{"embeddable":true,"href":"https:\/\/karmaka.de\/index.php?rest_route=%2Fwp%2Fv2%2Fcomments&post=17329"}],"version-history":[{"count":1,"href":"https:\/\/karmaka.de\/index.php?rest_route=\/wp\/v2\/posts\/17329\/revisions"}],"predecessor-version":[{"id":17330,"href":"https:\/\/karmaka.de\/index.php?rest_route=\/wp\/v2\/posts\/17329\/revisions\/17330"}],"wp:attachment":[{"href":"https:\/\/karmaka.de\/index.php?rest_route=%2Fwp%2Fv2%2Fmedia&parent=17329"}],"wp:term":[{"taxonomy":"category","embeddable":true,"href":"https:\/\/karmaka.de\/index.php?rest_route=%2Fwp%2Fv2%2Fcategories&post=17329"},{"taxonomy":"post_tag","embeddable":true,"href":"https:\/\/karmaka.de\/index.php?rest_route=%2Fwp%2Fv2%2Ftags&post=17329"}],"curies":[{"name":"wp","href":"https:\/\/api.w.org\/{rel}","templated":true}]}}